Tracklist: 1. Walker: Harlem Songs - 1. Spirituals 2. Walker: Harlem Songs - 2. Harlem Night Song 3. Walker: Harlem Songs - 3. Tambourines 4. Walker: God's Grandeur 5. Walker: An Hour To Dance - 1. Key Ring 6. Walker: An Hour To Dance - 2. Summary By The Prawns 7. Walker: An Hour To Dance - 3. The April Lovers 8. Walker: An Hour To Dance - 4. An Hour To Dance 9. Walker: An Hour To Dance - 5. Slow Scythe 10. Walker: An Hour To Dance - 6. White Darkness 11. Walker: An Hour To Dance - 7. Take My...
Source: CD
A duplicate t.p. apppears just before the Psalms
Topics: Bible, Hymns, Latin
Tracklist: 1. Walker: Harlem Songs - 1. Spirituals 2. Walker: Harlem Songs - 2. Harlem Night Song 3. Walker: Harlem Songs - 3. Tambourines 4. Walker: God's Grandeur 5. Walker: An Hour To Dance - 1. Key Ring 6. Walker: An Hour To Dance - 2. Summary By The Prawns 7. Walker: An Hour To Dance - 3. The April Lovers 8. Walker: An Hour To Dance - 4. An Hour To Dance 9. Walker: An Hour To Dance - 5. Slow Scythe 10. Walker: An Hour To Dance - 6. White Darkness 11. Walker: An Hour To Dance - 7. Take My...
Topic: Other Classical
Source: CD
39
39
Sep 19, 2013
09/13
by
Achim Bode; Urs M. Heller; Robert G. Edwards; Rajamani Narayanan
texts
eye 39
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We describe an HMC algorithm for dynamical overlap fermions which makes use of their good chiral properties. We test the algorithm in the Schwinger model. Topological sectors are readily changed even in the massless case.
Source: http://arxiv.org/abs/hep-lat/9912043v1
2
2.0
Jun 30, 2018
06/18
by
Valério A. R. M. Ribeiro; Michael F. Bode; Robert E. Williams
texts
eye 2
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comment 0
We modelled the late-time {\it Hubble Space Telescope} imaging of RS Ophiuchi with models from Ribeiro et al. (2009), which at the time due to the unknown availability of simultaneous ground-based spectroscopy left some open questions as to the evolution of the expanding nebular from the early to the late time observations. Initial emission line identifications suggest that no forbidden lines are present in the spectra and that the emission lines arising in the region of the WFPC2 F502N images...
Topics: Astrophysics, Solar and Stellar Astrophysics
Source: http://arxiv.org/abs/1410.0148
41
41
Sep 21, 2013
09/13
by
Andreja Gomboc; Shiho Kobayashi; Carole G. Mundell; Cristiano Guidorzi; Andrea Melandri; Iain A. Steele; Robert J. Smith; David Bersier; David Carter; Michael F. Bode; ;
texts
eye 41
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comment 0
Despite the pre-Swift expectation that bright optical flashes from reverse shocks would be prevalent in early-time afterglow emission, rapid response observations show this not to be the case. Although very bright at early times, some GRBs such as GRB 061007 and GRB 060418, lack the short-lived optical flash from the reverse shock within minutes after the GRB. In contrast, other optical afterglows, such as those of GRB 990123, GRB 021211, GRB 060111B, GRB 060117, GRB 061126, and recently GRB...
Source: http://arxiv.org/abs/0902.1830v2
32
32
Sep 22, 2013
09/13
by
Neta A. Bahcall; Feng Dong; Paul Bode; Rita Kim; James Annis; Timothy A. McKay; Sarah Hansen; James Gunn; Jeremiah P. Ostriker; Marc Postman; Robert C. Nichol; Tomotsugu Goto; Jon Brinkmann; Gillian R. Knapp; Don O. Lamb; Donald P. Schneider; Michael S. Vogeley; Donald G. York
texts
eye 32
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comment 0
The mass function of clusters of galaxies is determined from 400 deg^2 of early commissioning imaging data of the Sloan Digital Sky Survey; ~300 clusters in the redshift range z = 0.1 - 0.2 are used. Clusters are selected using two independent selection methods: a Matched Filter and a red-sequence color magnitude technique. The two methods yield consistent results. The cluster mass function is compared with large-scale cosmological simulations. We find a best-fit cluster normalization relation...
Source: http://arxiv.org/abs/astro-ph/0205490v2
71
71
Sep 21, 2013
09/13
by
Bradley E. Schaefer; Ashley Pagnotta; Aaron LaCluyze; Daniel E. Reichart; Kevin M. Ivarsen; Joshua B. Haislip; Melissa C. Nysewander; Justin P. Moore; Arto Oksanen; Hannah L. Worters; Ramotholo R. Sefako; Jaco Mentz; Shawn Dvorak; Tomas Gomez; Barbara G. Harris; Arne Henden; Thiam Guan Tan; Matthew Templeton; W. H. Allen; Berto Monard; Robert D. Rea; George Roberts; William Stein; Hiroyuki Maehara; Thomas Richards; Chris Stockdale; Tom Krajci; George Sjoberg; Jennie McCormick; Mikhail Revnivtsev; Sergei Molkov; Valery Suleimanov; Matthew J. Darnley; Michael F. Bode; Gerald Handler; Sebastien Lepine; Michael Shara
texts
eye 71
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comment 0
The eruption of the recurrent nova U Scorpii on 28 January 2010 is now the all-time best observed nova event. We report 36,776 magnitudes throughout its 67 day eruption, for an average of one measure every 2.6 minutes. This unique and unprecedented coverage is the first time that a nova has any substantial amount of fast photometry. With this, two new phenomena have been discovered: the fast flares in the early light curve seen from days 9-15 (which have no proposed explanation) and the optical...
Source: http://arxiv.org/abs/1108.1214v1
